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Facility/Payload OverviewMicrogravity Acceleration Measurement System (MAMS) studies the small forces, or vibrations and accelerations, on the International Space Station (ISS) that result from the operation of hardware, crew activities, dockings and maneuvering. Results are used to generalize the types of vibrations affecting vibration-sensitive experiments. Investigators seek to better understand the vibration environment on the space station.
Facility Manager(s)
Information Pending
Facility Developer
ZIN Technologies Incorporated, Cleveland, OH, United States
National Aeronautics and Space Administration (NASA)
Expeditions Assigned1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19/20, 21/22, 23/24, 25/26, 27/28, 29/30, 31/32, 33/34
Previous ISS MissionsMAMS has been operating on ISS since Expedition 2.
Changes in acceleration and moving mechanical parts cause small vibrations to move through the Station's structure. These disturbances occur within the frequency range of 0.01 to 300 Hz. Microgravity Acceleration Measurement System (MAMS) is one of two experiments onboard that measures and records the vibrations. The Space Acceleration Measurement System-II (SAMS-II) measures vibrations from vehicle acceleration, systems operations, and crew movements. MAMS complements this data by recording accelerations caused by aerodynamic drag and ISS movements caused by small attitude adjustments, gravity gradient, and the venting of water. These quasi-steady state accelerations occur in the frequency range below 1 Hz. MAMS consists of a low-frequency triaxial accelerometer, the Miniature Electro-Static Accelerometer (MESA), a high-frequency accelerometer, the High-Resolution Accelerometer Package (HiRAP), and associated computer, power, and signal processing subsystems contained within a Double Middeck Locker enclosure.
MESA consists of a hollow, cylindrical flanged mass, two X-axis forcing electrodes, an outer cylindrical proofmass carrier with Y- and Z-axis electrodes, and control electronics enclosed in a protective case. Static electricity forces the sensor proofmass to remain centered between the electrodes. The "sensed" acceleration is proportional to the voltage needed to keep the sensor centered.
MESA is mounted on a Bias Calibration Table Assembly (BCTA), a mechanism allowing on-orbit calibration. Calibration is used to remove electronic bias from the "sensed" acceleration.
Currently MAMS is only operated during special events such as an International Space Station (ISS) reboost and spacecraft dockings.
MAMS measures subtle accelerations that affect only certain types of experiments and is not operational all the time. MAMS operates from the Glenn Research Center Telescience Support Center at appropriate times. After initial installation on the Station, MAMS requires a minimum of four days of continuous operation to characterize the sensors' performance and to calculate any sensor bias. MAMS was set up and activated on May 8, 2001, and continued operation for eight days to collect data during normal Station operations. Since then, it has been reactivated several times to record dockings and other disturbances. Multiple calibrations taken over long periods of operation can be used to further improve the accuracy of MAMS data.
One of the major goals of the ISS is to provide a quiescent low-gravity environment to perform fundamental scientific research. However, small disturbances aboard the ISS impact the overall environment in which experiments are being performed. Such small disturbances need to be measured in order to assess their potential impact on the experiments. MAMS is used on board the ISS to do just that.
MAMS data have been analyzed to examine the quasi-steady regime on station with a frequency below 0.01 Hz. These are related to aerodynamic drag, gravity gradient and rotational effects, venting of air or water, and appendage movement, such as that of the solar arrays and antennas. Characteristics were found in the data that were unexplainable for a short period of time. Analysts determined that the movement of the Ku-band antenna was the source of the unusual characteristics in the quasi-steady data collected by MAMS. (A Ku-band antenna is used to transmit payload science data and video from ISS to Earth.) The correlation was made after comparing the data with real-time observations from ISS (DeLombard et al. 2002, 2004).
A special study using MAMS data was performed by ISS science officer Don Pettit during Expedition 6 as a part of Saturday Science. Pettit examined the motion of air bubbles in water to see how it correlated with quasi-steady accelerations, vibrations that are at or below a frequency of 0.01 Hz for a period greater than 100 seconds (DeLombard et al. 2005).
MAMS is currently being activated intermittently to meet operational requests for data during major mission events such as dockings by Soyuz and Progress vehicles. (Evans et al. 2009)
Information Pending
NASA Image: ISS003E6010 - Culbertson poses with MAMS hardware in the U.S. Laboratory during Expedition 3.
NASA Image: ISS007E06980 - Back-dropped by the blackness of space and Earth's horizon, an unmanned Progress supply vehicle approaches the ISS during Expedition 7. Inset image shows microgravity acceleration data provided by the MAMS hardware during a Progress docking with ISS.
NASA Image: ISS013E65575 - Shown is the Microgravity Acceleration Measurement System (MAMS) used to measure acceleration during specific ISS operations. MAMS is located in EXPRESS Rack 1 in the U.S. Laboratory.